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Diamond Infrared Emission Bands in Circumstellar Media

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Guillois, O., Ledoux, G., Reynaud, C.·1999·The Astrophysical Journal

Abstract

Since the discovery of small diamond grains in meteorites, the presence of such grains in the interstellar medium has been suspected. Here we report what we think to be the first unambiguous evidence of the presence of small crystallites of diamond in the dusty envelopes surrounding stars. Thanks to experimental results obtained in different laboratories on the diamond growth process, we identify two peculiar unidentified infrared emission bands at 3.43 and 3.53 μm as the vibrational modes of hydrogen-terminated crystalline facets of diamond. The intensities of these two strong features observed in the envelope of HD 97048 correspond to a mass of 10 -10 to 10 -9 M ☉ of diamond dust at an equilibrium temperature of ~1000 K.

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Metadata

Authors
Guillois, O., Ledoux, G., & Reynaud, C.
Venue
The Astrophysical Journal
Published
1999-08-20
Volume
521
Issue
2
Pages
L133-L136
ISSN
0004-637X (ISSN-L)
OpenAlex
W2080254629
Cited by
182
References
0
FWCI
6.34
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Diamond Infrared Emission Bands in Circumstellar Media. https://app.cochat.ai/papers/10.1086/312199
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Guillois, O., Ledoux, G., & Reynaud, C. (1999). Diamond Infrared Emission Bands in Circumstellar Media. The Astrophysical Journal. https://doi.org/10.1086/312199

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